The Sloan Digital Sky Survey-II Supernova Survey: Technical Summary
| dc.creator | Frieman, Joshua A. | |
| dc.creator | Bassett, B. | |
| dc.creator | Becker, A. | |
| dc.creator | Choi, C. | |
| dc.creator | Cinabro, D. | |
| dc.creator | DeJongh, F. | |
| dc.creator | Depoy, D. L. | |
| dc.creator | Dilday, B. | |
| dc.creator | Doi, M. | |
| dc.creator | Garnavich, P. M. | |
| dc.creator | Hogan, C. J. | |
| dc.creator | Holtzman, J. | |
| dc.creator | Im, M. | |
| dc.creator | Jha, S. | |
| dc.creator | Kessler, R. | |
| dc.creator | Konishi, K. | |
| dc.creator | Lampeitl, H. | |
| dc.creator | Marriner, J. | |
| dc.creator | Marshall, J. L. | |
| dc.creator | McGinnis, D. | |
| dc.creator | Miknaitis, G. | |
| dc.creator | Nichol, R. C. | |
| dc.creator | Prieto, J. L. | |
| dc.creator | Riess, A. G. | |
| dc.creator | Richmond, M. W. | |
| dc.creator | Romani, R. | |
| dc.creator | Sako, M. | |
| dc.creator | Schneider, D. P. | |
| dc.creator | Smith, M. | |
| dc.creator | Takanashi, N. | |
| dc.creator | Tokita, K. | |
| dc.creator | van der Heyden, K. | |
| dc.creator | Yasuda, N. | |
| dc.creator | Zheng, C. | |
| dc.creator | Adelman-McCarthy, J. | |
| dc.creator | Annis, J. | |
| dc.creator | Assef, R. J. | |
| dc.creator | Barentine, J. | |
| dc.creator | Bender, R. | |
| dc.creator | Blandford, R. D. | |
| dc.creator | Boroski, W. N. | |
| dc.creator | Bremer, M. | |
| dc.creator | Brewington, H. | |
| dc.creator | Collins, C. A. | |
| dc.creator | Crotts, A. | |
| dc.creator | Dembicky, J. | |
| dc.creator | Eastman, J. | |
| dc.creator | Edge, A. | |
| dc.creator | Edmondson, E. | |
| dc.creator | Elson, E. | |
| dc.creator | Eyler, M. E. | |
| dc.creator | Filippenko, A. V. | |
| dc.creator | Foley, R. J. | |
| dc.creator | Frank, S. | |
| dc.creator | Goobar, A. | |
| dc.creator | Gueth, T. | |
| dc.creator | Gunn, J. E. | |
| dc.creator | Harvanek, M. | |
| dc.creator | Hopp, U. | |
| dc.creator | Ihara, Y. | |
| dc.creator | Ivezić, Ž. | |
| dc.creator | Kahn, S. | |
| dc.creator | Kaplan, J. | |
| dc.creator | Kent, S. | |
| dc.creator | Ketzeback, W. | |
| dc.creator | Kleinman, S. J. | |
| dc.creator | Kollatschny, W. | |
| dc.creator | Kron, R. G. | |
| dc.creator | Krzesiński, J. | |
| dc.creator | Lamenti, D. | |
| dc.creator | Leloudas, G. | |
| dc.creator | Lin, H. | |
| dc.creator | Long, D. C. | |
| dc.creator | Lucey, J. | |
| dc.creator | Lupton, R. H. | |
| dc.creator | Malanushenko, E. | |
| dc.creator | Malanushenko, V. | |
| dc.creator | McMillan, R. J. | |
| dc.creator | Mendez, J. | |
| dc.creator | Morgan, C. W. | |
| dc.creator | Morokuma, T. | |
| dc.creator | Nitta, A. | |
| dc.creator | Ostman, L. | |
| dc.creator | Pan, K. | |
| dc.creator | Rockosi, C. M. | |
| dc.creator | Romer, A. K. | |
| dc.creator | Ruiz-Lapuente, P. | |
| dc.creator | Saurage, G. | |
| dc.creator | Schlesinger, K. | |
| dc.creator | Snedden, S. A. | |
| dc.creator | Sollerman, J. | |
| dc.creator | Stoughton, C. | |
| dc.creator | Stritzinger, M. | |
| dc.creator | SubbaRao, M. | |
| dc.creator | Tucker, D. | |
| dc.creator | Vaisanen, P. | |
| dc.creator | Watson, L. C. | |
| dc.creator | Watters, S. | |
| dc.creator | Wheeler, J. C. | |
| dc.creator | Yanny, B. | |
| dc.creator | York, D. | |
| dc.date | 2007-08-21 | |
| dc.date.accessioned | 2026-07-07T11:52:59Z | |
| dc.date.available | 2026-07-07T11:52:59Z | |
| dc.description | The Sloan Digital Sky Survey-II (SDSS-II) has embarked on a multi-year project to identify and measure light curves for intermediate-redshift (0.05 < z < 0.35) Type Ia supernovae (SNe Ia) using repeated five-band (ugriz) imaging over an area of 300 sq. deg. The survey region is a stripe 2.5 degrees wide centered on the celestial equator in the Southern Galactic Cap that has been imaged numerous times in earlier years, enabling construction of a deep reference image for discovery of new objects. Supernova imaging observations are being acquired between 1 September and 30 November of 2005-7. During the first two seasons, each region was imaged on average every five nights. Spectroscopic follow-up observations to determine supernova type and redshift are carried out on a large number of telescopes. In its first two three-month seasons, the survey has discovered and measured light curves for 327 spectroscopically confirmed SNe Ia, 30 probable SNe Ia, 14 confirmed SNe Ib/c, 32 confirmed SNe II, plus a large number of photometrically identified SNe Ia, 94 of which have host-galaxy spectra taken so far. This paper provides an overview of the project and briefly describes the observations completed during the first two seasons of operation. | |
| dc.description | Submitted to The Astronomical Journal (24 pages, 10 figures) | |
| dc.identifier | https://arxiv.org/abs/0708.2749 | |
| dc.identifier | http://arxiv.org/abs/0708.2749 | |
| dc.identifier | Astron.J.135:338-347,2008 | |
| dc.identifier | doi:10.1088/0004-6256/135/1/338 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/204378 | |
| dc.subject | Astrophysics | |
| dc.title | The Sloan Digital Sky Survey-II Supernova Survey: Technical Summary | |
| dc.type | text |